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| 1 | Progress in polar upper atmospheric physics research in China显示文摘The Chinese Antarctic Great Wall, Zhongshan, Kunlun and Arctic Yellow River stations have unique geographical locations, well suited to carry out polar upper atmospheric observations. This paper reviews the tremendous history of nearly 30 years of Chinese polar expeditions and major progress in polar upper atmospheric physics research. This includes the polar upper atmospheric physics conjugate observation system at Zhongshan Station in the Antarctic and Yellow River Station in the Arctic, and original research achievements in polar ionospheric fields, aurora and particle precipitation, the polar current system, polar plasma convection, geomagnetic pulsations and space plasma waves, inter-hemispheric comparisons of the space environment, space weather in polar regions, power spectrum of the incoherent scatter radar, ionospheric heating experiments and polar meso- spheric summer echoes, polar ionosphere-magnetosphere numerical simulation and others. Finally, prospects for Chinese polar upper atmospheric physics research are outlined. | LIU Ruiyuan YANG Huigen | 2012 | Advances in Polar Science2012，23，2： | 4 |
| 2 | 太阳活动区光球磁场特征的量化显示文摘为有效解决太阳活动区磁场特征量化问题,对所有SOHO卫星MDI磁图预处理后,分割出日面角45°以内的活动区,分析活动区投影面积变形来源,研究建立Cosine面积校正因子,校正活动区面积,构建具有21个特征参数的活动区磁场特征量化指标体系,通过主成分分析法对量化结果计算累积方差,结合活动区10486爆发X17.2级耀斑时的磁场变化定性分析。结果表明:强梯度极性分隔线权重磁场绝对值之和R、极性分隔线长度L_(PS)、强梯度极性分隔线长度L_(sg)和强梯度极性分隔线磁场绝对值之和Φ_(PSL)能够解释活动区磁场结构变化;磁场通量绝对值总和Φ_(uns)、磁场负通量总和Φ_(-)、磁场值代数和Φ_(tot)和磁场绝对值之和的平均值Φ_(mean)能够解释活动区磁场通量变化。Φ_(PSL)为本文新构建特征参数。上述参数可有效监测耀斑爆发前后活动区磁场结构和磁场通量的变化情况,量化结果可作为耀斑、质子事件监测及耀斑预报模型输入,为开展太阳爆发活动监测预警提供技术支撑。 | 杨晓华 王栖溪 夏仲飞 包赟 彭代亮 田天 徐龙 | 2022 | 空间科学学报2022，42，1： | 0 |
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